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首页> 外文期刊>Quarterly Journal of the Royal Meteorological Society >Assimilation of overcast cloudy infrared radiances of the geostationary MTSAT-1R imager
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Assimilation of overcast cloudy infrared radiances of the geostationary MTSAT-1R imager

机译:对地静止MTSAT-1R成像仪的阴天红外辐射的同化

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Infrared radiances from the Multi-functional Transport Satellite (MTSAT)-IR satellite were assimilated in cloudy conditions where effective cloud fractions were greater than 0.8. These cloudy radiances provide new information that currently assimilated clear-sky radiances from geostationary satellites and microwave sounders do not have. The radiance data to be assimilated were created by averaging pixels from the original radiances. We investigated how the characteristics of spatially averaged observations (super-observations or super-obs) vary with the super-ob size. The cloudy super-ob radiances were simulated by using a simple radiative transfer model with cloud-top pressure (P_c) and effective cloud fraction (N_e). The model assumed a single-layer cloud and that cloud emissivity does not depend on spectral wavelength. These two parameters were estimated by a minimum residual method with the infrared channel 1 (10.8 mum) and channel 2 (12.0 mum). To further ensure the validity of these assumptions, we limited use of super-ob radiances to almost completely overcast (N_e >0.8) conditions with homogeneous, middle to relatively high clouds (160 < P_c < 650 hPa). These overcast super-ob radiances (OSRs) from geostationary satellites have the advantages of (i) providing temperature information that is highly vertically resolved at the cloud top, (ii) providing frequent measurements, and (iii) being available in cloudy areas where clear radiances are often rejected by cloud quality-control procedures. Data assimilation experiments revealed that OSRs generally had a small impact on analyses and forecasts but provided a slightly improved forecast of temperatures in the upper troposphere and winds in the low troposphere.
机译:来自多功能运输卫星(MTSAT)-IR卫星的红外辐射在有效云量大于0.8的阴天条件下被吸收。这些多云的辐射提供了新的信息,这些信息目前没有吸收来自对地静止卫星和微波探测仪的晴空辐射。要吸收的辐射数据是通过对原始辐射的像素进行平均来创建的。我们研究了空间平均观测值(超观测值或超观测值)的特征如何随超观测值大小变化。通过使用具有云顶压力(P_c)和有效云分(N_e)的简单辐射传递模型,模拟了多云的超ob辐射。该模型假定为单层云,并且云发射率与光谱波长无关。这两个参数是通过最小残留方法使用红外通道1(10.8毫米)和通道2(12.0毫米)估算的。为了进一步确保这些假设的有效性,我们将超级ob辐射的使用范围限制在几乎完全阴(N_e> 0.8)的情况下,该云具有均匀,中等到相对较高的云(160

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